Thursday, April 25, 2024

Spring Moon (Camera/SharpCap Test?)

Seems like I am turning into a lunar photographer as of late since this is my second image within a month. Actually, like my last image, I was using the moon for testing once again. The moon is great for doing equipment and processing tests. In this case I was getting familiar with SharpCap again and testing my equipment for solar work.

My main solar setup consists of:
1) Orion ED80 - FL 600mm/F7.5
2) ZWO ASI178MM Pro
3) DayStar Quark Chromosphere
4) Orion Sirius Equatorial Mount
5) SharpCap capturing software

I used SharpCap to collect a video using the following camera settings:
Capture Area = 3096 x 2080
Gain = 290
Exposure = 0.2050ms
Duration = 20.189s
Frame Count = 496
Actual Frame Rate = 24.5680fps

I used AutoStakkert preprocessing processing software to stack the video frames selecting the best 20% or 99 frames. I did minimal final processing in PixInsight and Photoshop to produce this image. It came out pretty well but not as good as my single exposure shot from last month (https://www.astrobin.com/gv30xe/?nc=collection&nce=712). 

However, it is not really comparable since the slightest seeing conditions can affect the quality. Also, and maybe more important, they were with two completely different setups. Another thing that Niall MacNeill pointed out to me last month, was that lucky-stacking may work really well for closeup surface shots but for whole moon images single exposure shots show more detail. The following table lists the specs of each setup. Column 3 is my Solar Setup with the Quark and Column 4 is with the ASI174 (which I currently do not have) in place of the ASI178.


Edge800

ASI294MC

Solar Setup

ASI178

Solar Setup

w/Quark ASI178

Solar Setup

w/Quark ASI174

Telescope

Edge800

ED80

ED80

ED80

Reducer/Barlow

0.7x

none

4.2x

4.2x

Focal Length

1432mm

600mm

600mm

600mm

Camera

ASI294MC

ASI178MM

ASI178MM

ASI174MM

Pixel Size

4.63µm

2.4µm

2.4µm

5.86µm

Resolution

4144 x 2822

3096 x 2080

3096 x 2080

1936 x 1216

Sensor Size

19.1 x 13.1 mm

7.4 x 5.0 mm

7.4 x 5.0 mm

11.3 x 7.1 mm

Scale

0.67 arc”/pixel

0.83 arc”/pixel

0.2 arc”/pixel

0.48 arc”/pixel

Video Rate

19 fps 10bit/

16 fps 14bit

60 fps 10bit/

30 fps 14bit

60 fps 10bit/

30 fps 14bit

164 fps 10bit/

128 fps 12bit


The image scale are very close at 0.67 vs. 0.83 arcsec/pixel but there is no way to make up the difference between a 1432 mm Focal Length and a 600 mm Focal Length system. The whole point of using such a large scope is to get more detail.

The other thing I noticed was that the frame rate was ~24 fps which indicated that I was probably using 14 bit and for solar imaging it may be better to use 10 bit to take advantage of the higher capture rate. Of course I have no idea how to do this at the moment. Lastly, I may purchase the venerable ASI174 which has proven itself to be an excellent solar camera. It seems the price has come down a slight amount for that camera over the years most likely because ZWO has a newer and slightly more expensive solar camera, the ASI432.


Spring Moon (Camera/SharpCap Test?)
Date: 4-16-24
Camera: ZWO ASI178MM-Pro
Telescope: Orion ED80
Barlow: None
Focal Length: 600mm 
F/7.5
Focal Reducer: None
Mount: Orion Sirius Pro
Filter Adaptor: None
Filter: Camera UV-IR
Focuser: None
Autoguiding: None
Exposure: 99 x 0.2050 ms
Gain: 290
Offset 0
Temp: 15 C
Processing: SharpCap, AutoStakkert, PixInsight, Photoshop

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Monday, April 15, 2024

Barnard 35 (LBN 878 & 879)

Barnard 35 (B35) is a molecular cloud that is within the Lambda Orionis Ring (a.k.a Sh2-264) a huge molecular cloud and also a hydrogen alpha region located northwest of Betelgeuse in the Orion constellation. One of my favorite parts is LBN 878, the bright rim portion on the top where violent cosmic winds are blowing hydrogen (Ha) gas around. Herbig–Haro (HH) 175 is found in the bottom center of the rim (HH objects are associated with newborn stars). The bright yellow-brown reflection nebula known as GN 05.42.6 surrounds the young star FU Orionis. This lower brown region is known as LBN 879 or Ced 59. Distance to Barnard 35 assuming it is part of the Orion Molecular Cloud Complex is 1000 to 1400 light-years. The bottom right also has an interesting reflection portion rimmed in dense hydrogen gas (Ha).


I started imaged this in January imaging whenever it was clear and finished early March. I was originally more interested in an LRGB image with a bit of Ha but it only seemed to clear when the moon was out so I captured a lot of Ha and am glad I did. The most difficult part of processing was deciding what to bring out. From what I have seen, wide field images of this region accent the Ha whereas localized images focus on the reflection nebula. Although I was able to bring out a good deal of the reflection, my skies are not good enough facing the south to do reflection nebula justice - besides the Ha came out much better than I was expecting. I blended with the Ha and the LRGB until I wound up getting something I was happy with.

Hi Res: https://www.astrobin.com/vjujra/?nc=collection&nce=712

Dates: 1-14-24, 1-16, 1-17, 2-2, 2-3, 2-4, 2-5, 2-6, 2-7, 2-13, 2-14, 2-24, 2-25, 2-29, 3-3

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Barnard 35 (LBN 878 & 879)
Dates: 1-14-24, 1-16, 1-17, 2-2, 2-3, 2-4, 2-5, 2-6, 2-7, 2-13, 2-14, 2-24, 2-25, 2-29, 3-3
Camera: ZWO ASI1600MM-Pro
Telescope: Astro-Tech AT115EDT 115mm Refractor Telescope
Barlow: None
Focal Length: 805mm (644mm w/ FR)
f/7
Focal Reducer: 0.8x AstroTech Field Flatterner/Focal Reducer
Mount: Orion Sirius
Filter Wheel: ZWO
EFW 8 x 1.25"
Filter: Antlia Ha; ZWO L, R, G, B
Focuser: ZWO EAF
Autoguiding: ASI120 Mini attached to an Agena 50mm Guide Scope/ZWO 60mm Guidescope
Exposure: L 232 x 90, Ha 221 x 300, R 84 x 90, G 88 x 90, B 55 x 93 (Total 30h 50' 30")
Gain: 139
Offset 20
Sensor Temp: -20 C
Processing: NINA, PixInsight, Photoshop, BlurXTerminator, StarXTerminator, NoiseXTerminator, GraXpert, Bill Blanshan Color Masks, Bill Blanshan Stretching, Topaz Denoise.

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Wednesday, April 10, 2024

Eclipse 2024

Progression of the April 8, 2024 Eclipse from Dallas, Texas. After a cloudy morning and not so good weather report (thunderstorms later), the skies cleared a bit for the show! If you are wondering why I did not take a totality image, well there are so many other people doing that, no need, haha 😃. In reality, I should have done a meridian flip a couple of minutes prior to totality like I PLANNED. However, it was tracking so well I did not want to mess with it and figured it would track for a bit longer. It was completely my fault - the AM3 worked perfectly. I highly recommend this mount as it is super compact and not much bigger than a star tracker. The mount and tripod easily fits in carry-on luggage.

I did not try to hurry up to flip the mount and recenter because honestly observing the eclipse is so much more of a reward and I did not want to miss it. Besides, there are many excellent images of totality already and one more will not be missed. If you have never witnessed a total solar eclipse from totality, it is worth doing.


Eclipse 2024
Date: 4-8-24
Camera: Canon EOS Rebel T3i/600D modified
Telescope: Orion ST80
Barlow: None
Focal Length: 400mm
F/5
Focal Reducer: None,
Mount: ZWO AM3
Filter Adaptor: None
Filter(s): Astronomik OWB, SvBONY UV-IR
Focuser: None
Autoguiding: None
Exposure: white light 1/800s
ISO: 200
Offset 0
Temp: 24
Processing: PixInsight, Photoshop, BlurXT

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